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Prominences in SDO/EVE spectra: contributions from large solar structures

Published online by Cambridge University Press:  06 January 2014

Nicolas Labrosse ,
Hugh Hudson  and
Maria Kazachenko
Nicolas Labrosse
Affiliation:
SUPA, School of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, UK email: Nicolas.Labrosse@glasgow.ac.uk
Hugh Hudson
Affiliation:
SUPA, School of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, UK email: Nicolas.Labrosse@glasgow.ac.uk Space Sciences Laboratory, University of California, USA
Maria Kazachenko
Affiliation:
Space Sciences Laboratory, University of California, USA
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Abstract

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The EVE instrument on SDO is making accurate measurements of the solar spectral irradiance in the EUV between 30 and 1069 Å, with 1 Å spectral resolution and 10 s sampling rate. These data define solar variability in the “Sun-as-a-star” mode and reveal many interesting kinds of variation. Its high sensitivity also makes it suitable for spectroscopic diagnostics of solar features such as flares. Here we present EVE's potential contribution to the diagnostics of large-scale, slowly evolving features such as prominences and active regions, and what we can learn from this.

Keywords

Sun: activitySun: prominences
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S300: Nature of Prominences and their role in Space Weather , June 2013 , pp. 439 - 440
Copyright
Copyright © International Astronomical Union 2013